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Our knowledge about neutron star (NS) masses is renewed once again due to therecognition of the heaviest NS PSR J$ 0952-0607 $. By taking advantage of bothmass observations of super massive neutron stars and the tidal deformabilityderived from event GW170817, a joint constraint on tidal deformability isobtained. A wide-ranging correlation between NS pressure and tidaldeformability within the density range from saturation density $\rho_0$ to$5.6\rho_0$ is discovered, which directly yields a constrained NS EoS. Thenewly constrained EoS has a small uncertainty and a softer behavior at highdensities without the inclusion of extra degrees of freedom, which shows itspotential to be used as an indicator for the component of NS core.

PSR J$0952-0607$ and GW170817: Direct Multimessenger Constraints on Neutron Star Equation of State through a Novel Wide-ranging Correlation